The CANDELS/SHARDS Multiwavelength Catalog in GOODS-N: Photometry, Photometric Redshifts, Stellar Masses, Emission-line Fluxes, and Star Formation Rates

被引：150

作者：

Barro, Guillermo ^{[1
,2
]}

Perez-Gonzalez, Pablo G. ^{[3
,4
]}

Cava, Antonio ^{[5
]}

Brammer, Gabriel ^{[6
]}

Pandya, Viraj ^{[7
]}

Moral, Carmen Eliche ^{[8
]}

Esquej, Pilar ^{[9
]}

Dominguez-Sanchez, Helena ^{[10
]}

Alcalde Pampliega, Belen ^{[4
]}

Guo, Yicheng ^{[11
]}

Koekemoer, Anton M. ^{[6
]}

Trump, Jonathan R. ^{[12
]}

Ashby, Matthew L. N. ^{[13
]}

Cardiel, Nicolas ^{[4
]}

Castellano, Marco ^{[14
]}

Conselice, Christopher J. ^{[15
]}

Dickinson, Mark E. ^{[16
]}

Dolch, Timothy ^{[17
]}

Donley, Jennifer L. ^{[18
]}

Espino Briones, Nestor ^{[4
]}

Faber, Sandra M. ^{[7
]}

Fazio, Giovanni G. ^{[13
]}

Ferguson, Henry ^{[6
]}

Finkelstein, Steve ^{[19
]}

Fontana, Adrian ^{[14
]}

Galametz, Audrey ^{[20
]}

Gardner, Jonathan P. ^{[21
]}

Gawiser, Eric ^{[22
]}

Giavalisco, Mauro ^{[23
]}

Grazian, Andrea ^{[14
]}

Grogin, Norman A. ^{[6
]}

Hathi, Nimish P. ^{[6
]}

Hemmati, Shoubaneh ^{[24
]}

Hernan-Caballero, Antonio ^{[4
]}

Kocevski, Dale ^{[25
]}

Koo, David C. ^{[7
]}

Kodra, Dritan ^{[26
,27
]}

Lee, Kyoung-Soo ^{[28
]}

Lin, Lihwai ^{[29
]}

Lucas, Ray A. ^{[6
]}

Mobasher, Bahram ^{[30
]}

McGrath, Elizabeth J. ^{[25
]}

Nandra, Kirpal ^{[20
]}

Nayyeri, Hooshang ^{[31
]}

Newman, Jeffrey A. ^{[26
,27
]}

Pforr, Janine ^{[32
]}

Peth, Michael ^{[6
]}

Rafelski, Marc ^{[6
]}

Rodriguez-Munoz, Lucia ^{[33
]}

Salvato, Mara ^{[20
]}

机构：

[1] Univ Pacific, Stockton, CA 90340 USA

[2] Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA

[3] CSIC INTA, CAB, Ctr Astrobiol, Carretera Ajalvir Km 4, E-28850 Madrid, Spain

[4] Univ Complutense Madrid, F CC Fis, E-28040 Madrid, Spain

[5] Univ Geneva, Dept Astron, 51 Ch Maillettes, CH-1290 Versoix, Switzerland

[6] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[7] Univ Calif Santa Cruz, Dept Astron & Astrophys, UCO Lick Observ, Santa Cruz, CA 95064 USA

[8] Inst Astrofis Canarias, E-38200 Tenerife, Spain

[9] European Space Astron Ctr, E-28692 Madrid, Spain

[10] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[11] Univ Missouri, Dept Phys & Astron, Columbia, MO 65211 USA

[12] Univ Connecticut, Dept Phys, 2152 Hillside Rd,U-3046, Storrs, CT 06269 USA

[13] Harvard & Smithsonian, Ctr Astrophys, 60 Garden St,MS 66, Cambridge, MA 02138 USA

[14] INAF Osservatorio Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, RM, Italy

[15] Univ Nottingham, Sch Phys & Astron, Nottingham, England

[16] Natl Opt Astron Observ, 950 North Cherry Ave, Tucson, AZ 85719 USA

[17] Hillsdale Coll, Dept Phys, 33 E Coll St, Hillsdale, MI 49242 USA

[18] Los Alamos Natl Lab, Los Alamos, NM 87544 USA

[19] Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA

[20] Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr, D-85741 Garching, Germany

[21] NASA, Goddard Space Flight Ctr, Code 916, Greenbelt, MD 20771 USA

[22] Rutgers State Univ, Dept Phys & Astron, 136 Frelinghuysen Rd, Piscataway, NJ 08854 USA

[23] Univ Massachusetts, Dept Astron, 710 North Pleast St, Amherst, MA 01003 USA

[24] CALTECH, MS 100-22, Pasadena, CA 91125 USA

[25] Colby Coll, Dept Phys & Astron, Waterville, ME 04901 USA

[26] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA

[27] Univ Pittsburgh, PITT PACC, Pittsburgh, PA 15260 USA

[28] Purdue Univ, Dept Phys, 525 Northwestern Ave, W Lafayette, IN 47907 USA

[29] Acad Sinica, Inst Astron & Astrophys, Taipei 10617, Taiwan

[30] Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92521 USA

[31] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[32] European Space Technol Ctr, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands

[33] Univ Padua, Dipartimento Fis & Astron, Vicolo Osservatorio 3, Padua, Italy

[34] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[35] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[36] Catholic Univ Amer, Dept Phys, 620 Michigan Ave NE, Washington, DC 20064 USA

[37] Univ Bath, Dept Phys, Bath BA2 7AY, Avon, England

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2019年 / 243卷 / 02期

关键词：

galaxies: high-redshift; galaxies: photometry; DEEP-FIELD-SOUTH; SPECTRAL ENERGY-DISTRIBUTIONS; EARLY-TYPE GALAXIES; FORMATION HISTORY; SOURCE IDENTIFICATION; SPECTROSCOPIC SURVEY; LUMINOSITY FUNCTION; INFRARED PROPERTIES; FORMING GALAXIES; MASSIVE GALAXIES;

D O I：

10.3847/1538-4365/ab23f2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a WFC3 F160W (H-band) selected catalog in the CANDELS/GOODS-N field containing photometry from the ultraviolet (UV) to the far-infrared (IR), photometric redshifts, and stellar parameters derived from the analysis of the multiwavelength data. The catalog contains 35,445 sources over the 171 arcmin(2) of the CANDELS F160W mosaic. The 5 sigma detection limits (within an aperture of radius 0 ''.17) of the mosaic range between H = 27.8, 28.2, and 28.7 in the wide, intermediate, and deep regions, which span approximately 50%, 15%, and 35% of the total area. The multiwavelength photometry includes broadband data from the UV (U band from KPNO and LBC), optical (HST/ACS F435W, F606W, F775W, F814W, and F850LP), near-to-mid IR (HST/WFC3 F105W, F125W, F140W, and F160W; Subaru/MOIRCS Ks; CFHT/Megacam K; and Spitzer/IRAC 3.6, 4.5, 5.8, and 8.0 mu m), and far-IR (Spitzer/MIPS 24 mu m, HERSCHEL/PACS 100 and 160 mu m, SPIRE 250, 350 and 500 mu m) observations. In addition, the catalog also includes optical medium-band data (R similar to 50) in 25 consecutive bands, lambda = 500-950 nm, from the SHARDS survey and WFC3 IR spectroscopic observations with the G102 and G141 grisms (R similar to 210 and 130). The use of higher spectral resolution data to estimate photometric redshifts provides very high, and nearly uniform, precision from z = 0-2.5. The comparison to 1485 good-quality spectroscopic redshifts up to z similar to 3 yields Delta z/(1 + z(spec)) = 0.0032 and an outlier fraction of eta = 4.3%. In addition to the multiband photometry, we release value-added catalogs with emission-line fluxes, stellar masses, dust attenuations, UV- and IR-based star formation rates, and rest-frame colors.

引用

页数：41

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